| Revista: | Brazilian journal of physics |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000379548 |
| ISSN: | 0103-9733 |
| Autores: | Cao, Zhen1 |
| Instituciones: | 1Institute of High Energy Physics, Key Laboratory of Particle Astrophysics, Beijing. China |
| Año: | 2014 |
| Periodo: | Oct |
| Volumen: | 44 |
| Número: | 5 |
| Paginación: | 494-503 |
| País: | Brasil |
| Idioma: | Inglés |
| Tipo de documento: | Conferencia o discurso |
| Enfoque: | Analítico, descriptivo |
| Resumen en inglés | The ARGO-YBJ experiment in Tibet, China has been operated to survey the northern sky for gamma ray sources, transient or steady, for nearly 6 years. Many astrophysics observational results will be highlighted in this paper, such as the sky survey results, extended source observation, diffuse gamma rays from the galactic plane, and emission mechanism of AGNs and their flares. As the unique detector for EAS with a continuously sensitive area of 5,600 m2, the ARGO-YBJ array catches almost all particles in the central part of showers. The high-quality data set for showers above few TeV has been used for cosmic ray measurements such as the energy spectrum and composition. All those results are summarized here. As one of the next generation ground-based high-altitude air shower detector, LHAASO is briefly introduced as the successor of ARGO-YBJ in the end of the paper |
| Disciplinas: | Física y astronomía |
| Palabras clave: | Astronomía, Observaciones astrofísicas, Rayos gamma, Espectro de energía |
| Keyword: | Physics and astronomy, Astronomy, Astrophysical observations, Gamma rays, Energy spectrum |
| Texto completo: | Texto completo (Ver PDF) |
